activity
20042009
most citedMechanical First Law of Black Hole Spacetimes with Cosmological Constant and Its Application to Schwarzschild-de Sitter Spacetime

151 citations · 166 across the 5 of their papers we have counts for

collaborators

7 papers

gr-qc2009151 cited

Mechanical First Law of Black Hole Spacetimes with Cosmological Constant and Its Application to Schwarzschild-de Sitter Spacetime

Miho Urano, Akira Tomimatsu, Hiromi Saida

The mechanical first law (MFL) of black hole spacetimes is a geometrical relation which relates variations of mass parameter and horizon area. While it is well known that the MFL o…

astro-ph200810 cited

Constraints on the Evolution of Black Hole Spin due to Magnetohydrodynamic Accretion

Masaaki Takahashi, Akira Tomimatsu

Stationary and axisymmetric ideal magnetohydrodynamic (MHD) accretion onto a black hole is studied analytically. The accreting plasma ejected from a plasma source with low velocity…

gr-qc2006

Breakdown of self-similar evolution in homogeneous perfect fluid collapse

Eiji Mitsuda, Akira Tomimatsu

The stability analysis of self-similar solutions is an important approach to confirm whether they act as an attractor in general non-self-similar gravitational collapse. Assuming t…

gr-qc20062 cited

Stability analysis of self-similar behaviors in perfect fluid gravitational collapse

Eiji Mitsuda, Akira Tomimatsu

Stability of self-similar solutions for gravitational collapse is an important problem to be investigated from the perspectives of their nature as an attractor, critical phenomena…

gr-qc2005

Distortion of Schwarzschild-anti-de Sitter black holes to black strings

A. Tomimatsu

Motivated by the existence of black holes with various topologies in four-dimensional spacetimes with a negative cosmological constant, we study axisymmetric static solutions descr…

gr-qc20053 cited

Electromagnetic radiation due to naked singularity formation in self-similar gravitational collapse

Eiji Mitsuda, Hirotaka Yoshino, Akira Tomimatsu

Dynamical evolution of test fields in background geometry with a naked singularity is an important problem relevant to the Cauchy horizon instability and the observational signatur…